Reexploration of interacting holographic dark energy model: cases of interaction term excluding the Hubble parameter

Author:

Li Hai-Li,Zhang Jing-Fei,Feng Lu,Zhang Xin

Funder

National Natural Science Foundation of China

Publisher

Springer Science and Business Media LLC

Subject

Physics and Astronomy (miscellaneous),Engineering (miscellaneous)

Reference134 articles.

1. A.G. Riess et al. [Supernova Search Team Collaboration], Observational evidence from supernovae for an accelerating universe and a cosmological constant. Astron. J. 116, 1009 (1998) arXiv:astro-ph/9805201

2. S. Perlmutter et al. [Supernova Cosmology Project Collaboration], Measurements of Omega and Lambda from 42 high redshift supernovae. Astrophys. J. 517, 565 (1999). arXiv:astro-ph/9812133

3. D.N. Spergel et al. [WMAP Collaboration], First year Wilkinson microwave anisotropy probe (WMAP) observations: determination of cosmological parameters. Astrophys. J. Suppl. 148, 175 (2003). arXiv:astro-ph/0302209

4. C.L. Bennett et al. [WMAP Collaboration], First year Wilkinson microwave anisotropy probe (WMAP) observations: preliminary maps and basic results. Astrophys. J. Suppl. 148, 1 (2003). arXiv:astro-ph/0302207

5. M. Tegmark et al. [SDSS Collaboration], Cosmological parameters from SDSS and WMAP. Phys. Rev. D 69, 103501 (2004). arXiv:astro-ph/0310723

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